12 Ophiuchi is avariable star 32.3light-years away in theconstellationOphiuchus. No companions have yet been detected in orbit around this star, and it remains uncertain whether or not it possesses a dust ring.[8]
This star is categorized as aBY Draconis variable, with variable star designation V2133. The variability is attributed to large-scale magnetic activity on thechromosphere (in the form ofstarspots) combined with a rotational period that moved the active regions into (and out of) the line of sight. This results in low amplitude variability of 12 Ophiuchi's luminosity. The star also appears to display rapid variation in luminosity, possibly due to changes in the starspots.[9] Measurements of the long-term variability show two overlapping cycles of starspot activity (compared to the Sun's single, 11-year cycle.) The periods of these two cycles are 4.0 and 17.4 years.[10]
Its abundance of heavy elements (elements heavier thanhelium) is nearly identical to that of the Sun. The surface gravity is equal to, which is somewhat higher than the Sun's.[4] The space velocity is 30 km/s relative to the Solar System. The high rotation period and active chromosphere are indicative of a relatively young star.[12][13]
^Houk, N.; Swift, C. (1999), "Michigan catalogue of two-dimensional spectral types for the HD Stars",Michigan Spectral Survey,5,Bibcode:1999MSS...C05....0H.
^H. J. Habing; P. Bouchet; C. Dominik;T. Encrenaz; A. Heske; M. Jourdain de Muizon; et al. (1996). "First results from a photometric infrared survey for Vega-like disks around nearby main-sequence stars".Astronomy and Astrophysics.315:L233 –L236.Bibcode:1996A&A...315L.233H.
^J. D. Dorren; E. F. Guinan; E. F. (1982). "Evidence for starspots on single solar-like stars".Astronomical Journal.87:1546–1557.Bibcode:1982AJ.....87.1546D.doi:10.1086/113245.
